\begin{table}%t2 %\centering \par \caption{\label{tab2}Summary of the results obtained for the entire population of microlenses towards the LMC for the EROS experiment, using models~A, B and~C and adopting an age of the halo of 14~Gyr and several magnitude cuts.} \begin{tabular}{lrrrrrrrrrrrrr} \hline \hline\noalign{\smallskip} \multicolumn{1}{c} {\ } &\multicolumn{4}{c}{Model A} &\multicolumn{4}{c}{Model B} &\multicolumn{4}{c}{Model C}\\ \hline Magnitude & 17.5 & 22.5 & 27.5 & 32.5 & 17.5 & 22.5 & 27.5 & 32.5 & 17.5 & 22.5 & 27.5 & 32.5 \\ \cline{2-5} \cline{6-9} \cline{10-13} \\ $\langle N_{\rm WD}\rangle$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$\\ $\langle N_{\rm RD}\rangle$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$ & $0\pm1$\\ $\langle m_{\rm WD}\rangle$ $(M/M_{\sun})$ & 0.383 & 0.601 & 0.618 & 0.744 & 0.602 & 0.598 & 0.621 & 0.674 & 0.590 & 0.605 & 0.610 & 0.666 \\ $\langle m_{\rm RD}\rangle$ $(M/M_{\sun})$ & 0.328 & 0.206 & 0.111 & 0.083 & 0.305 & 0.208 & 0.118 & 0.082 & 0.304 & 0.177 & 0.112 & 0.085 \\ $\langle\eta\rangle$ & 0.186 & 0.246 & 0.373 & 0.671 & 0.774 & 0.800 & 0.919 & 0.965 & 0.711 & 0.882 & 0.957 & 0.976 \\ $\langle \mu\rangle\;(''~{\rm yr}^{-1})$ & 0.021 & 0.017 & 0.009 & 0.006 & 0.022 & 0.016 & 0.016 & 0.015 & 0.021 & 0.017 & 0.011 & 0.016 \\ $\langle d\rangle$ (kpc) & 2.51 & 3.16 & 5.52 & 9.04 & 2.46 & 3.35 & 3.58 & 3.80 & 2.56 & 3.23 & 4.83 & 3.21 \\ $\langle V_{\rm tan} \rangle\; ({\rm km~s}^{-1})$ & 250 & 258 & 244 & 245 & 254 & 259 & 272 & 275 & 261 & 257 & 259 & 245 \\ $\langle\hat{t}_{\rm E}\rangle $ (d) & 41.9 & 44.1 & 60.7 & 88.8 & 35.9 & 40.9 & 43.5 & 53.2 & 38.1 & 39.6 & 49.4 & 63.9 \\ $\langle\tau/\tau_0\rangle$ & 0.977 & 0.810 & 0.659 & 0.384 & 0.794 & 0.678 & 0.400 & 0.214 & 0.775 & 0.618 & 0.352 & 0.259 \\ \hline \end{tabular} \end{table}